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In this contribution, I discuss some of the salient features of L and T dwarf spectra in both the red optical (6300–10000 {\AA}) and near-infrared (1–2.5 ) wavelength regimes. Important absorption bands and lines, including those of HO, CH, FeH, CrH, CO, and the alkali metal lines, are identified, and the development of recent classification schemes based on these features are discussed. I briefly point out future work required in these wavelength regions and in the mid-infrared that are required to garner a complete picture of these low-luminosity dwarfs.

生成讲解博客的中文版本

生成AI智能校验的中文版本